... Arithmetic Functions . Random Numbers . String Conversion . Searching and Sorting . ... There are 4 basic integer functions: . int abs(int number); long int labs(long int number); div_t div(int numerator,int denominator); ldiv_t ldiv(long int numerator, long int denominator); . ... In practice no functions produce truly random data -- they produce pseudo-random numbers. ... The stdlib.h provides 2 useful functions to perform general searching and sorting of data on any type. ...

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• Time Functions
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SLR Observations at the Quasar Network Stations I.Gayazov, V.Mitryaev, S.Smolentsev, I.Rahimov, A.Diyakov, V.Shpilevski, V.Pshenkin, Ya.Rets Institute of Applied Astronomy, Saint Petersburg, Russia WPLTN-2012 September 24 - 28, 2012 Saint Petersburg SLR systems installation at the Quasar observatories Observatory Zelenchukskaya Badary Stage Dome building System installation Testing Dome building System installation Testing Dome building ...

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• Stellarium: AngleSpinBox Class Reference
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OptInt PmWiki : Pm Wiki / Basic Variables . ... Defaults to 'AsSpaced'. ... Defaults to 'Profiles'. ... If {$FullName} is "Group.Page-Draft" then {$BaseName} is "Group.Page" $BaseNamePatterns['/-Draft$/'] = ''; # If {$FullName} is "Comments-Group.Page" then {$BaseName} is "Group.Page" $BaseNamePatterns['/^Comments-/'] = ''; . ... WikiGroup used by default (on startup) when no group is specified in the URL, as in "Main". ... Can be used to override the default date format used by the "ftime" function. ...

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• OptInt PmWiki : PmWiki / Wiki Style Examples
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• Bojan Nikolic -- Simple smoothing of astronomical images in FITS format

function [P,T0]= lafkin ( file , ncol ,pmin,pmax, ncycl , Ydir ); % % % % Function call: [P,T0]= lafkin ( file , ncol ,pmin,pmax, ncycl , Ydir ); % OR % lafkin ( file , ncol ,pmin,pmax, ncycl , Ydir ); % % Datafile structure: % 1st column - JD % 2 ,3 ,4, ..., columns - data to process (light, color, rad. vel. curves) % % Input: file - filename (write as 'V001.DAT') % ...

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• jg0025
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Magnetic Stars, 2011, pp. ... 2008). ... The origin of magnetic fields of hot massive stars is explained by the fossil field theory, MAGNETISM OF STARS 451 1-5 Be measurements -> 1278 stars 100 N stars 6-10 Be measurements -> 80 stars 50 11-15 Be measurements -> 47 stars 0 20 40 60 80 100 120 140 160 180 The namber of individual measurements The number of individual measurements Figure 1: The number of stars in a single bin versus the number of individual Be determinations for a single star. ...

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• http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p476.pdf
• SAO RAS - Telescopes - BTA - MSS
• UGC 2172, NGC 3239

A descriptor , also commonly called a file handle is an object that a program uses to read or write an open file, or open network socket, or a variety of other devices. ... The operating system enforces a limit on the number of descriptors that a program can have open at a time. ... One is a kernel limitation, depending on your operating system you will either be able to tune the number of descriptors available to higher numbers (this is frequently called FD_SETSIZE ). ...

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• Running a High-Performance Web Server for BSD
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. Произведение и частное двух чисел . число A: число B: .

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• Model realization and some results
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... 2. (a) Metallicity function and relations between (b) metallicity and radial velocity, (c) metallicity and maximum distance from the Galactic plane,and (d)metallicity and variability period for RR Lyrae variables in the initial sample.The curve in the first graph is the maximum-likelihood approximation of the distribution using a sum of two normal curves with the indicated means,dispersions,and total numbers. ... next figure | privious figure . ...

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• F-stars in galactic disk, figures
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• Vladimir Marsakov Publication List

. Russian Version [ MS-Win ] . [ News ] . [ Satellite data ] . [ SMIS ] . [ ] . The program processes multi-band images to detect homogeneous areas and perform image classification. It includes a number of segmentation algorithms. The classification can be performed using various methods - nearest neighbor, normalized distance, estimate calculation. Demo version . Price . Back to SMIS Home Page .

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• Myasnyankin Andrey , Moscow Institute of Physics and Technology (MIPT),Space
• Matyushkin Evgeny, Space Research Institute (SRI)
• XV-IMAGE

... Sunspot Region 30 . ... The solar active region designated number 0030 is now appearing on the visible hemisphere of the closest star. Dwarfed by the Sun's disk, the group of sunspots which make up region 30 actually cover an enormous area -- nearly 10 times the size of Earth. ... The star cluster in RCW38 was hiding. ... The reason is that the open cluster is so young that it is still shrouded in thick dust that absorbs visible light. ... Proxima Centauri: The Closest Star . ...

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... 1 A80 Model number and parameters (in model.dat file) 3- 6 A80 Self explanatory header 7 A80 Bolometric linear coefficients 9- 376 A80 Law coefficients 378-73891 A80 Repeating the above for the 195 models -------------------------------------------------------------------------- ... ------------------------------------------------------------------------- 1- 10 A10 --- bolometric comment 12- 18 F7.3 --- xLin coefficient of the linear ...

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• Astronomical Catalogues
• SAO Star Catalog
• Positions and Proper Motions

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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December 16, 1997 . ... An example of the EUV chain revealed by the modified SOHO/EIT images. A complex EUV (195 A) chain or thread of December 16, 1997, consisting of several quasi-straight-line fragments between points 1-2-3-4-5 and covering a large part of the solar disk. ... A comparison of the large-scale chains and threads on two pairs of the modified SOHO/EIT (195 A; inverted) and He I (10830 A; normal) images. ... SOHO/EIT, 195 A, December 15-17, 1997 GIF Animation (1.07 MB) . ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20151005.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150704.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2014/obzor20140303.en.txt

... Thermogravimetric and differential thermal analysis . Electrode polarization measurements . ... Total conductivity, Seebeck coefficient and ion transference number measurements in controlled atmos . ... Processing of ceramic materials, electrode systems and electrochemical cells . Synthesis of solid oxide materials for high-temperature electrochemical applications . ... 4-probe DC conductivity measurements in controlled atmospheres, combined with Seebeck coefficient determination. ...

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• LPCBC: Abstract, 2_6
• Teams at the International Astronomy Olympiad
• Theoretical department of ISSP RAS

... Each file has a header and number of data records. ... -23) 2 I3 Minute (0-59) 3 I3 Second (0-59) 4 I4 Millisecond 5 F3.0 Code F/S (1,2,3,4,5) Defines the pair of the electromagnetic field components measured, see Table 2.1 6 A3 Electromagnetic field component measured in the filters ACP1-ACP5 (BX, BX45 ,BZ,EH,EZ) 7 E11.3 Field Intensity in the Filter ACP1 nT/ sqrt (Hz) if BX, BX45 , or BZ; V/ m.sqrt (Hz) if EH, or EZ 8 E9.3 Field Intensity in the Filter ACP2 nT/ ...

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• Identities
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... Behemoth black hole found in an unlikely place . ... black holes . ... Observing springtime deep-sky objects with a large telescope . ... Could large numbers of black holes account for much of the "dark matter" estimated to exist in our universe? ... NASA, ESA, M.J. Jee and H. Ford (Johns Hopkins University) No, because the universe never had the raw material to grow enough black holes to account for current estimates of dark matter. Get instant access to subscriber content on Astronomy.com! ...

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• The right number of images | Astronomy.com
• Carry around the universe's top numbers | Astronomy.com
• Discovery triples the number of stars in the universe | Astronomy.com

. [ A | B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z ] . a unique number associated with each filename. This number is used to look up an entry in the inode table which gives information on the type, size, and location of the file and the userid of the owner of the file.

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• rtftohtml Users Guide - 1 An Overview of rtftohtml
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... Peter B. Mozhaev , Ph.D. Complicated crystal structure and anisotropy of physical properties of the high critical temperature superconductors (HTSC) makes difficult reproducible fabrication of the multilayered epitaxial heterostructures of HTSC with necessary parameters. ... The goal of this project is study of growth and formation of the multilayer epitaxial heterostructures of HTSC of the ReBa 2 Cu 3 O x family (ReBCO, where Re is the rare earth element). ...

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• Project 8 - RFBR - Dynamical and non-equilibrium electron transport and
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... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• LINN?, a Software System for Automatic Classification
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
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